1RXP J113123+4322.5: post-outburst modulations During March 16, 17, and 18, the object is gradually fading at a rate of 0.14mag/d. Our period analysis using these post-outburst light curves provided the best period of 0.0643(2) d, slightly shorter than the superhump period during the superoutburst. The average light curve show two peaks; one is probably associated with ordinary superhumps (amplitude ~0.1mag), and the other is late superhumps (~0.5mag). Time-series observations are still encouraged to monitor the evolution of these humps and possible rebrightenings. Regards, Makoto Uemura